Science in Short ChaptersWilliams, W. Mattieu (William Mattieu)
Science
Science in Short Chapters
Williams, W. Mattieu (William Mattieu)
Science
I make this digression in order to repudiate any participation in
this kind of speculation. Though “The Fuel of the Sun” is avowedly a
very bold attempt to unravel majestic mysteries, I have not sought
_to elucidate the known by means of the unknown_, as do these
inventors of imaginary agents, but have scrupulously followed the
opposite principle. I have invented nothing, but have started from
the experimental facts of the laboratory, the demonstrated laws of
physical action, and have followed up step by step what I understand
to be the necessary consequences of these. Many years ago I convinced
myself that our atmosphere is but a portion of universal atmospheric
matter; that Dr. Wollaston was wrong, and that the compression of this
universal atmospheric matter is possibly the source of solar light
and heat; but as this was long before M. Deville had investigated
the subject of dissociation by heat,[6] I was unable to work out
the problem at all satisfactorily. When I subsequently resumed the
subject, I knew nothing about the corona, and had only read of the “red
prominences” as possible lunar appendages, or solar clouds, or optical
illusions. I had worked out the necessity of the gaseous eruptions,
and their action in effecting an interchange of solar and general
atmospheric matter, as the means of maintaining the solar light and
heat, with no idea of proceeding further with the problem, when the
announcement that the prominences were not merely unquestionable solar
appendages, but were actually upheaved mountains of glowing hydrogen,
suddenly and unexpectedly suggested their identity with my required
atmospheric upheavals. It is true that their observed magnitude far
exceeded my theoretical anticipations, and in this respect I have made
some _à posteriori_ adaptations, especially with the aid of a clearer
understanding of the laws of dissociation which almost simultaneously
became attainable.
In like manner, the necessity of the solid ejections presented
themselves before I knew anything of the recently discovered details of
the coronal phenomena—when I had merely read of a luminous halo which
had been seen around the sun, and relying upon Mr. Lockyer, vaguely
supposed it to be an effect of atmospheric illumination. I inferred
that streams of solid particles must be pouring from the sun, and
showering back again, but had no idea that such streams and showers
were actually visible until I was rather startled on learning that the
corona, instead of being, as I had loosely supposed, a mere uniform
filmy halo, had been described by Mr. De la Rue, in his Bakerian
Lecture on the Eclipse of 1860, as “softening off with very irregular
outline, and sending off some _long streams_,” etc. I was then living
on the sides of a Welsh mountain far away from public libraries, and
being no astronomer, my own books kept me better acquainted with the
current progress of experimental than with astronomical science.
Public-domain text, read in full here on John Shaqi.
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